CO2 Phase Changes and Flow Mechanisms for Non-Aqueous ``Floods'' on Mars

Details CO2 Phase Changes and Flow Mechanisms for Non-Aqueous ``Floods'' on Mars CO2 Phase Changes and Flow Mechanisms for Non-Aqueous ``Floods'' on Mars

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001lpi....32.1288h&link_type=abstract

32nd Annual Lunar and Planetary Science Conference, March 12-16, 2001, Houston, Texas, abstract no.1288

Physics

Scientific paper

Water is not required as the active medium for sediment transport and
erosion in the outburst 'floods'. CO2 vapour-supported density flows are
an ideal and far more probable mechanism. Explosive outbursts of
subsurface liquid CO2 fuel the flows.

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